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Understanding the radio emission geometry of multi-component radio pulsars from retardation and aberration effects

ASTROPHYSICAL JOURNAL, no. 1 (2003): 418-426

Cited: 70|Views29

Abstract

We have conducted a detailed analysis of the emission geometry of a handful of radio pulsars that have prominent, multiple-component profiles at meter wavelengths. From careful determination of the total number of emission components and their locations in pulse longitude, we find that all of the six pulsars show clear evidence for retard...More

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